Showing 1–20 of 32 results
/ Date/ Name
Mar 23, 2026Reinterpreting the puzzling properties of z>6 galaxies within a variable IMF frameworkFeb 26, 2026Extreme Emission Line Galaxies in CEERS Are Powered by Star Formation, not AGNFeb 24, 2026Simulations of the 21cm emission line for upcoming large-scale HI galaxy surveysFeb 23, 2026Little Red Dots: One Photometric Tag Concealing Diverse Spectroscopic Flavors of Massive Star Formation and Black Hole ActivityDec 14, 2025THRILS -- The High-(Redshift+Ionization) Line Search: Program Description & Redshift CatalogNov 24, 2025Beyond the Monsters: A More Complete Census of Black Hole Activity at Cosmic DawnNov 19, 2025Do z>6 quasars reside in protoclusters?Nov 11, 2025Where Giants Dwell: Probing the Environments of Early Massive Quiescent GalaxiesOct 14, 2025A census of quiescent galaxies across $0.5 < z < 8$ with JWST/MIRI: Mass-dependent number density evolution of quiescent galaxies in the early UniverseSep 4, 2025Characterizing the roles of transitory obscured phases and inner torus in shaping the fractions of obscured AGN at cosmic noonJul 3, 2025Testing Photometric Techniques for Measuring the Rest-Frame UV Spectral Slope Against JWST PRISM SpectroscopyJun 26, 2025Optical Strong Line Ratios Cannot Distinguish Between Stellar Populations and Accreting Black Holes at High Ionization Parameters and Low MetallicitiesMay 7, 2025CAPERS-LRD-z9: A Gas Enshrouded Little Red Dot Hosting a Broad-line AGN at z=9.288Apr 17, 2025The impact of ram pressure on cluster galaxies, insights from GAEA and TNGApr 16, 2025CAPERS Observations of Two UV-Bright Galaxies at z>10. More Evidence for Bursting Star Formation in the Early UniverseFeb 5, 2025Emission-Line Diagnostics at z>4: [OIII]λ4363/HγFeb 3, 2025Cosmic quenchingJan 7, 2025The Cosmic Evolution Early Release Science Survey (CEERS)Oct 9, 2024Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their HostsSep 10, 2024Broad-Line AGN at 3.5<z<6: The Black Hole Mass Function and a Connection with Little Red Dots